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• W2161796271 abstract "It is crucial to identify the ultrahigh-energy cosmic-ray (UHECR) sources and probe their unknown properties. Recent results from the Pierre Auger Observatory favor a heavy nuclear composition for the UHECRs. Under the requirement that heavy nuclei survive in these sources, using gamma-ray bursts as an example, we predict a diagnostic gamma-ray signal, unique to nuclei - the emission of de-excitation gamma rays following photodisintegration. These gamma rays, boosted from MeV to TeV-PeV energies, may be detectable by gamma-ray telescopes such as VERITAS, HESS, and MAGIC, and especially the next-generation CTA and AGIS. They are a promising messenger to identify and study individual UHE nuclei accelerators." @default.
• W2161796271 created "2016-06-24" @default.
• W2161796271 creator A5007068870 @default.
• W2161796271 creator A5068174431 @default.
• W2161796271 date "2010-08-19" @default.
• W2161796271 modified "2023-10-06" @default.
• W2161796271 title "Very-high-energy gamma-ray signal from nuclear photodisintegration as a probe of extragalactic sources of ultrahigh-energy nuclei" @default.
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• W2161796271 doi "https://doi.org/10.1103/physrevd.82.043008" @default.
• W2161796271 hasPublicationYear "2010" @default.
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